Dunes on Titan observed by Cassini Radar
WALL, S. D.
Jet Propulsion Laboratory [JPL]
Laboratoire de Planétologie et Géodynamique [UMR 6112] [LPG]
Jet Propulsion Laboratory [JPL]
Laboratoire de Planétologie et Géodynamique [UMR 6112] [LPG]
LOPES, R. M.
Jet Propulsion Laboratory [JPL]
Therapies Interventionnelles Assistees Par l'Image et la Simulation - U 703 [Thiais]
Jet Propulsion Laboratory [JPL]
Therapies Interventionnelles Assistees Par l'Image et la Simulation - U 703 [Thiais]
PAILLOU, Philippe
Laboratoire d'astrodynamique, d'astrophysique et d'aéronomie de bordeaux [L3AB]
Observatoire aquitain des sciences de l'univers [OASU]
Laboratoire d'Astrophysique de Bordeaux [Pessac] [LAB]
Laboratoire de l'intégration, du matériau au système [IMS]
< Leer menos
Laboratoire d'astrodynamique, d'astrophysique et d'aéronomie de bordeaux [L3AB]
Observatoire aquitain des sciences de l'univers [OASU]
Laboratoire d'Astrophysique de Bordeaux [Pessac] [LAB]
Laboratoire de l'intégration, du matériau au système [IMS]
Idioma
en
Article de revue
Este ítem está publicado en
Icarus. 2008, vol. 194, n° 2, p. 690-703
Elsevier
Resumen en inglés
Thousands of longitudinal dunes have recently been discovered by the Titan Radar Mapper on the surface of Titan. These are found mainly within ±30° of the equator in optically-, near-infrared-, and radar-dark regions, ...Leer más >
Thousands of longitudinal dunes have recently been discovered by the Titan Radar Mapper on the surface of Titan. These are found mainly within ±30° of the equator in optically-, near-infrared-, and radar-dark regions, indicating a strong proportion of organics, and cover well over 5% of Titan's surface. Their longitudinal duneform, interactions with topography, and correlation with other aeolian forms indicate a single, dominant wind direction aligned with the dune axis plus lesser, off-axis or seasonally alternating winds. Global compilations of dune orientations reveal the mean wind direction is dominantly eastwards, with regional and local variations where winds are diverted around topographically high features, such as mountain blocks or broad landforms. Global winds may carry sediments from high latitude regions to equatorial regions, where relatively drier conditions prevail, and the particles are reworked into dunes, perhaps on timescales of thousands to tens of thousands of years. On Titan, adequate sediment supply, sufficient wind, and the absence of sediment carriage and trapping by fluids are the dominant factors in the presence of dunes.< Leer menos
Palabras clave
Titan
surfaces
Saturn
satellites
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